Imidazolium-Catalyzed Synthesis of an Imidazolium Catalyst.

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY Origins of Life and Evolution of Biospheres Pub Date : 2019-12-01 Epub Date: 2019-12-08 DOI:10.1007/s11084-019-09589-2
Arthur L Weber, Andro C Rios
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Abstract

The chemistry of imidazolium-catalyzed imidazolium synthesis was studied as part of an effort to develop a plausible prebiotic synthesis of a small catalytic molecule capable of catalyzing its own synthesis. Specifically, we investigated the one-pot 1-ethyl-3-methylimidazolium acetate (EMIM-Ac) catalyzed synthesis of 1,3-dibutyl-4,5-difuryl-imidazolium acetate (DBDFIM-Ac) from furfural, n-butylamine, formaldehyde, and acetic acid at 80 °C. Liu et al. (2012) had previously demonstrated the first reaction of the synthetic process, the EMIM-Ac catalyzed benzoin condensation of furfural that yields furoin. Our early studies established the second reaction of the synthetic process, the multicomponent reaction of furoin, n-butylamine, formaldehyde, and acetic acid that yields the imidazolium salt, DBDFIM-Ac. Studies of the complete two-reaction process that uses furfural for the synthesis of DBDFIM-Ac showed that the highest yield of DBDFIM-Ac was obtained when the mole ratio of n-butylamine, formaldehyde, and acetic acid relative to furfural was respectively (0.5:0.25:0.25:1.0-furfural), or one-half of the stoichiometric ratio (1.0:0.5:0.5:1.0-furfural). A time course study of the process showed transient formation of furoin, the obligatory reaction intermediate. DBDFIM-Ac and the imidazolium side product, 1,3-dibutyl-4,5-trifuryl-imidazolium acetate (DBTFIM-Ac), were stable under the reaction conditions. Imidazolium products (DBDFIM and DBTFIM) and the furoin intermediate were not formed in control reactions (80 °C, 24 h) in which EMIM catalyst was either absent or replaced with an equal volume of acetonitrile or DMF. The imidazolium product, DBDFIM-Ac, was shown to catalyze the synthesis of structurally similar 1,3-dipentyl-4,5-difuryl-imidazolium acetate (DPDFIM-Ac) from furfural, n-pentylamine, formaldehyde, and acetic acid at 80 °C.

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咪唑催化合成一种咪唑催化剂。
我们研究了咪唑鎓催化咪唑鎓合成的化学过程,作为开发一种能够催化自身合成的小催化分子的似是而非的预生物合成方法的努力的一部分。具体来说,我们研究了在 80 °C下由糠醛、正丁胺、甲醛和乙酸催化合成 1,3-二丁基-4,5-二糠基咪唑鎓乙酸盐(DBDFIM-Ac)的一锅式 1-乙基-3-甲基咪唑鎓乙酸盐(EMIM-Ac)。Liu 等人(2012 年)之前已经证明了合成过程的第一个反应,即 EMIM-Ac 催化糠醛的安息香缩合反应生成呋喃西林。我们的早期研究确定了合成过程的第二个反应,即呋喃、正丁胺、甲醛和乙酸的多组分反应,生成咪唑盐 DBDFIM-Ac。对使用糠醛合成 DBDFIM-Ac 的完整双反应过程的研究表明,当正丁胺、甲醛和乙酸相对于糠醛的摩尔比分别为(0.5:0.25:0.25:1.0-糠醛)或化学计量比(1.0:0.5:0.5:1.0-糠醛)的二分之一时,DBDFIM-Ac 的产量最高。对这一过程的时程研究表明,呋喃醛是瞬时形成的必经反应中间体。DBDFIM-Ac 和咪唑鎓副产物 1,3-二丁基-4,5-三硫基咪唑鎓乙酸酯(DBTFIM-Ac)在反应条件下是稳定的。在不使用 EMIM 催化剂或用等体积乙腈或 DMF 取代 EMIM 催化剂的对照反应(80 °C,24 小时)中,没有形成咪唑鎓产物(DBDFIM 和 DBTFIM)和呋喃中间体。研究表明,咪唑产物 DBDFIM-Ac 可在 80 ℃ 下催化糠醛、正戊胺、甲醛和乙酸合成结构相似的 1,3-二戊基-4,5-二糠基咪唑鎓乙酸盐 (DPDFIM-Ac)。
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来源期刊
CiteScore
3.20
自引率
15.00%
发文量
12
审稿时长
>12 weeks
期刊介绍: The subject of the origin and early evolution of life is an inseparable part of the general discipline of Astrobiology. The journal Origins of Life and Evolution of Biospheres places special importance on the interconnection as well as the interdisciplinary nature of these fields, as is reflected in its subject coverage. While any scientific study which contributes to our understanding of the origins, evolution and distribution of life in the Universe is suitable for inclusion in the journal, some examples of important areas of interest are: prebiotic chemistry and the nature of Earth''s early environment, self-replicating and self-organizing systems, the theory of the RNA world and of other possible precursor systems, and the problem of the origin of the genetic code. Early evolution of life - as revealed by such techniques as the elucidation of biochemical pathways, molecular phylogeny, the study of Precambrian sediments and fossils and of major innovations in microbial evolution - forms a second focus. As a larger and more general context for these areas, Astrobiology refers to the origin and evolution of life in a cosmic setting, and includes interstellar chemistry, planetary atmospheres and habitable zones, the organic chemistry of comets, meteorites, asteroids and other small bodies, biological adaptation to extreme environments, life detection and related areas. Experimental papers, theoretical articles and authorative literature reviews are all appropriate forms for submission to the journal. In the coming years, Astrobiology will play an even greater role in defining the journal''s coverage and keeping Origins of Life and Evolution of Biospheres well-placed in this growing interdisciplinary field.
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